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arXiv 0804.2328hep-phastro-phnucl-th
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天体物理对约束模型的约束:场关联函数方法

Astrophysical constraints on the confining models : the Field Correlator Method

M. Baldo, G. F. Burgio, P. Castorina, S. Plumari, D. Zappala'

摘要:

我们探讨了禁闭的相关性,在夸克物质模型的可能夸克核心的中子星。对于夸克相位,我们采用了由场关联函数方法导出的状态方程,并将其推广到零温极限。对于强子相,我们使用微观Brueckner-Hartree-Fock多体理论。我们发现,目前采用的值的胶子凝聚$G_2 \simeq 0.006-0.007 \rm {GeV^4}$,它给出了一个临界温度$T_c \simeq 170 \rm MeV$,产生最大的质量,这是只有轻微的观测极限一致,而更大的质量是可能的,如果胶子凝聚增加。

英文摘要:

We explore the relevance of confinement in quark matter models for the possible quark core of neutron stars. For the quark phase, we adopt the equation of state (EoS) derived with the Field Correlator Method, extended to the zero temperature limit. For the hadronic phase, we use the microscopic Brueckner-Hartree-Fock many-body theory. We find that the currently adopted value of the gluon condensate $G_2 \simeq 0.006-0.007 \rm {GeV^4}$, which gives a critical temperature $T_c \simeq 170 \rm MeV$, produces maximum masses which are only marginally consistent with the observational limit, while larger masses are possible if the gluon condensate is increased.

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